Results 1 to 10 of about 2,175 (190)

Outflowing Helium from a Mature Mini-Neptune [PDF]

open access: goldThe Astrophysical Journal Letters, 2023
We announce the detection of escaping helium from TOI 2134b, a mini-Neptune a few gigayears old. The average in-transit absorption spectrum shows a peak of 0.37% ± 0.05% and an equivalent width of W _avg = 3.3 ± 0.3 mÅ.
Michael Zhang   +4 more
doaj   +4 more sources

Detection of Atmospheric Escape from Four Young Mini-Neptunes [PDF]

open access: goldThe Astronomical Journal, 2023
We use Keck/NIRSPEC to survey a sample of of young (
Michael Zhang   +7 more
doaj   +5 more sources

A Mini-Neptune Orbiting the Metal-poor K Dwarf BD+29 2654 [PDF]

open access: greenThe Astronomical Journal, 2023
We report the discovery and Doppler mass measurement of a 7.4 days 2.3 R _⊕ mini-Neptune around a metal-poor K dwarf BD+29 2654 (TOI-2018). Based on a high-resolution Keck/HIRES spectrum, the Gaia parallax, and multiwavelength photometry from the UV to ...
Fei Dai   +50 more
doaj   +7 more sources

The formation of mini-Neptunes [PDF]

open access: bronzeThe Astrophysical Journal, 2017
Mini-Neptunes seem to be common planets. In this work we investigate the possible formation histories and predicted occurrence rates of mini-Neptunes assuming the planets form beyond the iceline.
Helled, Ravit, Venturini, Julia
core   +5 more sources

Distinguishing Oceans of Water from Magma on Mini-Neptune K2-18b [PDF]

open access: greenThe Astrophysical Journal Letters
Mildly irradiated mini-Neptunes have densities potentially consistent with them hosting substantial liquid-water oceans (“Hycean” planets). The presence of CO _2 and simultaneous absence of ammonia (NH _3 ) in their atmospheres has been proposed as a ...
Oliver Shorttle   +4 more
doaj   +7 more sources

Evolutionary Models of Super-Earths and Mini-Neptunes Incorporating Cooling and Mass Loss [PDF]

open access: greenThe Astrophysical Journal, 2015
We construct models of the structural evolution of super-Earth- and mini-Neptune-type exoplanets with hydrogen-helium envelopes, incorporating radiative cooling and XUV-driven mass loss.
Burrows, Adam S., Howe, Alex R.
core   +4 more sources

Kepler and the Behemoth: Three Mini-Neptunes in a 40 Million Year Old Association [PDF]

open access: goldThe Astronomical Journal, 2022
Stellar positions and velocities from Gaia are yielding a new view of open cluster dispersal. Here we present an analysis of a group of stars spanning Cepheus ( l = 100°) to Hercules ( l = 40°), hereafter the Cep-Her complex.
L. G. Bouma   +10 more
doaj   +4 more sources

JWST Observations of K2-18b Can Be Explained by a Gas-rich Mini-Neptune with No Habitable Surface [PDF]

open access: goldThe Astrophysical Journal Letters
The James Webb Space Telescope (JWST) recently measured the transmission spectrum of K2-18b, a habitable-zone sub-Neptune exoplanet, detecting CH _4 and CO _2 in its atmosphere.
Nicholas F. Wogan   +5 more
doaj   +4 more sources

Occurrence and core-envelope structure of 1-4× Earth-size planets around Sun-like stars. [PDF]

open access: yesProc Natl Acad Sci U S A, 2014
Small planets, 1-4x the size of Earth, are extremely common around Sun-like stars, and surprisingly so, as they are missing in our solar system. Recent detections have yielded enough information about this class of exoplanets to begin characterizing ...
Marcy GW   +5 more
europepmc   +4 more sources

Habitable Evaporated Cores: Transforming Mini-Neptunes into Super-Earths in the Habitable Zones of M Dwarfs [PDF]

open access: green, 2015
We show that photoevaporation of small gaseous exoplanets ("mini-Neptunes") in the habitable zones of M dwarfs can remove several Earth masses of hydrogen and helium from these planets and transform them into potentially habitable worlds. We couple X-ray/
Barnes, Rory   +5 more
core   +2 more sources

Home - About - Disclaimer - Privacy